\begin{table}%tA.1
\caption{The local sample: Seyfert 1.0 to 1.5, narrow line Seyfert 1s (NLS1) and broad line radio galaxies (BLRGs).}
%\centering
\par
\begin{tabular}{lcccrcrcc}
\hline \hline \noalign{\smallskip}
Name& Type& $z$& log~$N_{\rm H}$& log~$f_{2-10}$& ${\rm Ref}_{\rm X}$& log~$f_{\rm NeV}$& A& $\rm Ref_{NeV}$\\
(1)& (2)& (3)& (4)& (5)& (6)& (7)& (8)& (9)\\ 
\hline
       NGC~3227&   1.5&  0.0039&   22.83& --11.09&  1&  --13.05&  L&   1\\ 
       NGC~3516&   1.5&  0.0088&   20.63& --10.62&  2&  --13.15&  L&   1\\ 
       NGC~3783&   1.0&  0.0097&   20.00& --10.07&  3&  --12.86&  M&   2\\ 
       NGC~4051&   1.5&  0.0020&   20.00& --10.64&  4&  --12.98&  L&   1\\ 
       NGC~4151&   1.5&  0.0033&   22.88& --10.35&  1&  --11.70&  L&   1\\ 
       NGC~4253&  NLS1&  0.0129&   20.00& --10.80&  5&  --13.49&  M&   3\\ 
       NGC~4395&   1.0&  0.0010&   20.80& --11.30&  6&  --14.10&  S&   4\\ 
       NGC~4593&   1.0&  0.0090&   20.00& --10.43&  7&  --13.60&  M&   2\\ 
       NGC~5548&   1.5&  0.0172&   20.00& --10.28&  7&  --12.57&  L&   1\\ 
       NGC~6814&   1.5&  0.0052&   20.00& --11.82&  8&  --13.77&  M&   2\\ 
       NGC~7469&   1.2&  0.0163&   20.00& --10.64&  7&  --12.74&  L&   1\\ 
         Mrk~42&  NLS1&  0.0246&   20.00& --11.98&  9&  --14.52&  L&   5\\ 
        Mrk~359&  NLS1&  0.0169&   20.00& --11.24&  10&  --13.30&  S&   4\\ 
        Mrk~486&  NLS1&  0.0389&   20.00& --11.55&  11&  --13.68&  S&   4\\ 
        Mrk~493&  NLS1&  0.0313&   20.00& --11.46&  10&  --14.52&  M&   3\\ 
        Mrk~509&   1.2&  0.0344&   20.00& --10.47&  7&  --12.24&  M&   2\\ 
        Mrk~704&   1.5&  0.0291&   23.13& --11.25&  12&  --13.21&  S&   4\\ 
        Mrk~705&   1.2&  0.0285&   20.00& --10.64&  13&  --13.80&  S&   4\\ 
        Mrk~841&   1.5&  0.0364&   20.00& --10.79&  14&  --13.15&  M&   2\\ 
        Mrk~896&   1.0&  0.0264&   20.00& --11.46&  10&  --14.10&  M&   2\\ 
        Mrk~926&   1.5&  0.0469&   20.00& --10.51&  7&  --13.96&  S&  6\\ 
       Mrk~1239&  NLS1&  0.0194&   23.52& --11.82&  15&  --13.31&  S&   4\\ 
         3C~120&  BLRG&  0.0330&   20.70& --10.31&  16&  --13.72&  S&  6\\ 
         3C~227&  BLRG&  0.0858&   22.10& --11.70&  17&  --14.40&  M&  7\\ 
         3C~382&  BLRG&  0.0578&   20.00& --10.21&  18&  --13.85&  M&  7\\ 
       3C~390.3&  BLRG&  0.0561&   20.60& --10.40&  19&  --13.59&  S&   4\\ 
         3C~445&  BLRG&  0.0562&   22.70& --11.17&  20&  --13.85&  M&   2\\ 
      Fairall~9&   1.2&  0.0470&   20.00& --10.92&  7&  --13.03&  M&   8\\ 
     Fairall~51&   1.0&  0.0142&   22.20& --10.60&  21&  --13.29&  M&   2\\ 
   Fairall~1116&   1.0&  0.0582&   20.00& --11.27&  22&  --13.54&  M&   8\\ 
   Tol~1351-375&   1.9&  0.0520&   22.20& --11.42&  23&  --13.48&  M&   2\\ 
  Tol~1506.3-00&   1.5&  0.0543&   21.85& --11.11&  24&  --14.00&  M&   2\\ 
     H1143-182&   1.5&  0.0329&   20.00& --10.55&  4&  --13.19&  M&   8\\ 
     H1846-786&   1.0&  0.0743&   20.00& --11.10&  7&  --13.49&  M&   2\\ 
        Akn~120&   1.0&  0.0330&   20.00& --10.42&  25&  --14.15&  S&   4\\ 
        Akn~564&  NLS1&  0.0247&   20.00& --10.80&  26&  --13.33&  S&   4\\ 
   MCG-6-30-15&   1.2&  0.0077&   20.00& --10.62&  27&  --14.05&  M&   2\\ 
   1ES1615+061&   1.5&  0.0380&   20.00& --11.10&  28&  --14.22&  M&   2\\ 
       IIIZw77&   1.2&  0.0342&   23.90& --12.22&  24&  --13.55&  M&  9\\ 
    ESO~141-G55&   1.2&  0.0360&   20.00& --10.57&  29&  --13.17&  M&  8\\ 
         POX~52&   1.0&  0.0218&   20.70& --12.11&  30&  --13.35&  M&  10\\ 
\hline		 	      			\end{tabular}
\tablefoot {Column description: (1) Source name. (2) Spectroscopic classification (1.0, 1.2 and 1.5 refer to Seyfert types). (3) Redshift. (4) Logarithm of the cold X-ray absorbing column density. For those objects in which no cold absorption is measured in excess of the Galactic value, the
column has been fixed to log~$N_{\rm H}$~= 20. (5) Logarithm of the observed 2$-$10~keV flux in erg~cm$^{-2}$~s$^{-1}$. (6) Reference for the X-ray data. (7) Logarithm of the [Ne~V]3426 flux in erg~cm$^{-2}$~s$^{-1}$. (8) Aperture used to measure the [Ne~V] flux, defined following Schmitt (1998): S (small), M (medium) and L (large) correspond to apertures in the ranges 1$-$3$''$, 3$-$7$''$, and  $>$7$''$, respectively. (9) Reference for the [Ne~V] data. \\
{\it X-ray references}: (1) \citet{cappi06}; (2) \citet{bianchi04}; (3) \citet{blustin02}; (4) \citet{bianchi09};  (5) \citet{landi05}; (6)~\citet{iwa10}; (7) \citet{shinozaki06}; (8) \citet{vf07}; (9) \citet{vaughan99}; (10) \citet{gallo06}; (11) \citet{ballo08}; (12) \citet{landi07}; (13) \citet{gallo05}; (14) \citet{pico05}; (15) \citet{grupe04}; (16) \citet{grandi06}; (17)~\citet{hard07}; (18) \citet{gliozzi07}; (19) \citet{evans06}; (20) \citet{sambruna07}; (21) \citet{jime08} (22)~\citet{dammando08}; (23) \citet{guido00}; (24) this work;  (25) \citet{vaughan04}; (26) \citet{vignali04}; (27) \citet{ponti04}; (28) \citet{guainazzi98}; (29) \citet{gondoin03}; (30) \citet{thornton08}. \\
{\it [Ne~V] references}: (1) \citet{anderson70}; (2) \citet{mw88}; (3) \citet{op85}; 
(4) \citet{erkens97};  (5) \citet{malkan86}; (6) \citet{db88}; 
(7) \citet{o76}; (8) \citet{winkler92}; (9) \citet{o81iii}; (10) \citet{kunth87}.}
\vspace*{0.7mm}
\end{table}